activity
20102023
most citedPhantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics

431 citations · 3.2k across the 62 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

astro-ph.SR2018★ 7 cited

On the role of magnetic fields in star formation

C. J. Nixon, J. E. Pringle

Magnetic fields are observed in star forming regions. However simulations of the late stages of star formation that do not include magnetic fields provide a good fit to the propert…

astro-ph.HE2018★ 19 cited

Circumbinary discs around merging stellar-mass black holes

Rebecca G. Martin, Chris Nixon, Fu-Guo Xie +1

A circumbinary disc around a pair of merging stellar-mass black holes may be shocked and heated during the recoil of the merged hole, causing a near-simultaneous electromagnetic co…

astro-ph.EP2018★ 64 cited

Warping a protoplanetary disc with a planet on an inclined orbit

Rebecca Nealon, Giovanni Dipierro, Richard Alexander +2

Recent observations of several protoplanetary discs have found evidence of departures from flat, circular motion in the inner regions of the disc. One possible explanation for thes…

astro-ph.SR2018★ 13 cited

The galactic rate of second and third generation disc and planet formation

Miriam Hogg, Graham Wynn, Chris Nixon

We investigate the formation of discs within binary systems where at least one component has left the main sequence. In particular we calculate the occurrence rates of systems whic…

astro-ph.HE2018★ 57 cited

Super-Eddington Accretion in Tidal Disruption Events: the Impact of Realistic Fallback Rates on Accretion Rates

Samantha Wu, Eric R. Coughlin, Chris Nixon

After the tidal disruption of a star by a massive black hole, disrupted stellar debris can fall back to the hole at a rate significantly exceeding its Eddington limit. To understan…

astro-ph.HE2018★ 18 cited

Misaligned Accretion and Jet Production

Andrew King, Chris Nixon

Disc accretion on to a black hole is often misaligned from its spin axis. If the disc maintains a significant magnetic field normal to its local plane, we show that dipole radiatio…

astro-ph.GA2018★ 12 cited

The origin of the structure of large-scale magnetic fields in disc galaxies

C. J. Nixon, T. O. Hands, A. R. King +1

The large-scale magnetic fields observed in spiral disc galaxies are often thought to result from dynamo action in the disc plane. However, the increasing importance of Faraday dep…